| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1770868 | Astroparticle Physics | 2012 | 30 Pages |
Abstract
⺠We propose a 3-stage DM and IË1/2 observatory based on multi-ton LXe and LAr detectors. ⺠This work is a quantitative study of the topics in Astropart. Phys. 31 (2009) 63-74. ⺠WIMP cross-sections and masses could be measured with sensitivity of 10-47cm2. ⺠0ν2β decay could be observed for 136Xe with sensitivity to half-lives 10E27-10E28 y. ⺠The pp solar ν spectrum, and ν flux from a Galactic SN, could also be measured.
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Authors
K. Arisaka, P. Beltrame, C.W. Lam, P.F. Smith, C. Ghag, D.B. Cline, K. Lung, Y. Meng, E. Pantic, P.R. Scovell, A. Teymourian,